Detached eclipsing binaries (dEBs) are our primary source of measurements of the physical properties of normal stars [1]}, [2]} and have many astrophysical applications [1]}, [4]}, [5]}. dEBs containing stars of similar mass to our Sun are useful in particular in helping to constrain our understanding of stellar theory in the mass regime around the solar fiducial point, for example the amounts of internal mixing and convective core overshooting [6]}, [7]}, [8]}. Solar-type dEBs can also be helpful in studying starspot configurations [9]}, [10]}, [11]} and the radius discrepancy whereby low-mass stars are found to be systematically larger and cooler than predicted by theoretical models [6]}, [13]}, [14]}.
